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I review extant methods for estimating star formation rates across the electromagnetic spectrum, comparing extragalactic with Galactic (Milky Way) estimators. Present (GALEX, Spitzer) and future (Herschel, JWST) space facilities have opened new windows or increased sensitivity in old ones for measuring star formation rates in both local and distant galaxies. This important parameter not only is key to the investigation of galaxy evolution, but provides insights into the physics of star formation in galaxies. For the latter, the upcoming Large Millimeter Telescope will set the stage for the exploration of the new frontier. I finally review the outlook from the point of view of recently approved Herschel Key Projects.
Colloquia are usually preceded by coffee and followed by an informal reception (both in room CSS 0254). Anyone interested in having lunch or talking with the speaker should contact either of the colloquium coordinators (see below). The hour immediately after lunch will normally be reserved for the speaker to talk to graduate students. Students are urged to contact the coordinator to arrange this.
Request colloquia announcements by e-mail:
coll-request@astro.umd.edu
Colloquium Organizer:
Andrew Wilson (301) 405-1519
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Department of Astronomy, University of Maryland College Park, MD 20742-2421 Phone: (301) 405-3001 FAX: (301) 314-9067 Comments and questions may be directed to webmaster@astro.umd.edu
This page was automatically generated on:
20-Feb-2008.
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